ARG0000fyb - is the edge-on spiral the host of the extended radio emission?
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by JeanTate
SDSS J130143.51+525327.2, with z_sp 0.033, is quite local. It's also a disk galaxy, possibly a bulgeless one:
Is it the host of the FIRST radio emission, with the weird morphology?
Or is it, perhaps, the STAR SDSS J130142.71+525330.4?
Boilerplate: SDSS image per
http://skyservice.pha.jhu.edu/DR10/ImgCutout/getjpeg.aspx
, FIRST (red) contours derived from the FITS file produced using SkyView with Python code described in this RGZ Talk thread. Image center (J2000.0) is the galaxy SDSS J130143.51+525327.2; "z_sp" its SDSS spectroscopic redshift.Posted
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by JeanTate in response to JeanTate's comment.
Zooming out a bit, and adding NVSS:
Does rather look like a doublelobe ... but what's the host?
Boilerplate: SDSS image per
http://skyservice.pha.jhu.edu/DR10/ImgCutout/getjpeg.aspx
, FIRST (red) and NVSS (cyan) contours derived from FITS files produced using SkyView with Python code described in this RGZ Talk thread. Image center (J2000.0) is the galaxy SDSS J130143.51+525327.2; "z_sp" its SDSS spectroscopic redshift.Posted